GCN Circular 2367

K. Hurley and T. Cline, on behalf of the Ulysses and Konus GRB teams,

E. Mazets and S. Golenetskii, on behalf of the Konus-Wind GRB team,

A. von Kienlin, G. Lichti, and A. Rau, on behalf of the INTEGRAL
SPI-ACS GRB team, and

G. Ricker, J-L Atteia, N. Kawai, D. Lamb, S. Woosley, J. Doty, R.
Vanderspek, J. Villasenor, G. Crew, G. Monnelly, N. Butler, J.G.
Jernigan, A. Levine, F. Martel, E. Morgan, G. Prigozhin, J. Braga, R.
Manchanda, G.  Pizzichini, Y. Shirasaki, C. Graziani, M. Matsuoka, T.
Tamagawa, K. Torii, T. Sakamoto, A. Yoshida, E. Fenimore, M. Galassi,
T. Tavenner, T.  Donaghy, M. Boer, J-F Olive, and J-P Dezalay, on
behalf of the HETE GRB team, report:

Ulysses, Konus-Wind, INTEGRAL (SPI-ACS), and HETE (FREGATE)  observed
this GRB at 67228 seconds.  As observed by Ulysses, it had a duration
of approximately 10 seconds, a 25-100 keV fluence of approximately
2E-06 erg/cm2, and a peak flux of approximately  7.4E-07 erg/cm2 s over
0.25 seconds.

We have triangulated it to a preliminary annulus centered  at RA,
Decl(2000)= 341.187, -22.949 degrees, whose radius is 76.591 +/-  0.143
degrees (3 sigma).

This annulus can be constrained and/or improved, but as the event was
not observed by Mars Odyssey, a small error box cannot be derived for
it.